French Katherine L, Hallmann Christian, Hope Janet M, Schoon Petra L, Zumberge J Alex, Hoshino Yosuke, Peters Carl A, George Simon C, Love Gordon D, Brocks Jochen J, Buick Roger, Summons Roger E
Joint Program in Chemical Oceanography, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution, Cambridge, MA 02139;
Max Planck Institute for Biogeochemistry, 07745 Jena, Germany; Center for Marine Environmental Sciences, University of Bremen, 28359 Bremen, Germany;
Proc Natl Acad Sci U S A. 2015 May 12;112(19):5915-20. doi: 10.1073/pnas.1419563112. Epub 2015 Apr 27.
Hopanes and steranes found in Archean rocks have been presented as key evidence supporting the early rise of oxygenic photosynthesis and eukaryotes, but the syngeneity of these hydrocarbon biomarkers is controversial. To resolve this debate, we performed a multilaboratory study of new cores from the Pilbara Craton, Australia, that were drilled and sampled using unprecedented hydrocarbon-clean protocols. Hopanes and steranes in rock extracts and hydropyrolysates from these new cores were typically at or below our femtogram detection limit, but when they were detectable, they had total hopane (<37.9 pg per gram of rock) and total sterane (<32.9 pg per gram of rock) concentrations comparable to those measured in blanks and negative control samples. In contrast, hopanes and steranes measured in the exteriors of conventionally drilled and curated rocks of stratigraphic equivalence reach concentrations of 389.5 pg per gram of rock and 1,039 pg per gram of rock, respectively. Polycyclic aromatic hydrocarbons and diamondoids, which exceed blank concentrations, exhibit individual concentrations up to 80 ng per gram of rock in rock extracts and up to 1,000 ng per gram of rock in hydropyrolysates from the ultraclean cores. These results demonstrate that previously studied Archean samples host mixtures of biomarker contaminants and indigenous overmature hydrocarbons. Therefore, existing lipid biomarker evidence cannot be invoked to support the emergence of oxygenic photosynthesis and eukaryotes by ∼ 2.7 billion years ago. Although suitable Proterozoic rocks exist, no currently known Archean strata lie within the appropriate thermal maturity window for syngenetic hydrocarbon biomarker preservation, so future exploration for Archean biomarkers should screen for rocks with milder thermal histories.
在太古宙岩石中发现的藿烷类和甾烷类物质被视为支持早期氧光合作用和真核生物兴起的关键证据,但这些碳氢化合物生物标志物的同生性存在争议。为解决这一争论,我们对来自澳大利亚皮尔巴拉克拉通的新岩芯进行了多实验室研究,这些岩芯是采用前所未有的碳氢化合物清洁方案进行钻探和采样的。这些新岩芯的岩石提取物和加氢热解产物中的藿烷类和甾烷类物质通常处于或低于我们的飞克检测限,但当它们可被检测到时,其总藿烷(每克岩石<37.9皮克)和总甾烷(每克岩石<32.9皮克)浓度与在空白和阴性对照样品中测得的浓度相当。相比之下,在具有地层等效性的传统钻探和保存的岩石外部测得的藿烷类和甾烷类物质浓度分别达到每克岩石389.5皮克和每克岩石1039皮克。多环芳烃和类金刚石,其浓度超过空白浓度,在超清洁岩芯的岩石提取物中个别浓度高达每克岩石80纳克,在加氢热解产物中高达每克岩石1000纳克。这些结果表明,先前研究的太古宙样品含有生物标志物污染物和原生过成熟碳氢化合物的混合物。因此,现有的脂质生物标志物证据不能用来支持约27亿年前氧光合作用和真核生物的出现。尽管存在合适的元古宙岩石,但目前已知的太古宙地层都不在适合同生碳氢化合物生物标志物保存的热成熟窗口内,因此未来对太古宙生物标志物的探索应筛选热历史较温和的岩石。